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hal.structure.identifierECLIPSE 2018
dc.contributor.authorBOUTIN-BASILLAIS, B.
hal.structure.identifierECLIPSE 2018
dc.contributor.authorHURÉ, J.-M.
dc.date.issued2018
dc.date.conference2018-07-03
dc.description.abstractEnWe present an efficient multi-body code devoted to self-gravitating polytropic stars and rings in mutual gravitational interaction. The code implements the Self-Consistent Field method which captures solutions in an iterative manner. It works for any positive polytropic index, rotation law and configuration (axis ratios and relative separations). The number of bodies is free. We have investigated a wide range of equilibria involving 2 up to 8 bodies. A model for the disk around HL Tau is currently under progress.
dc.language.isoen
dc.subject.enMethods: numerical
dc.subject.enStars: rotation
dc.subject.enEquation of state
dc.subject.enGravitation
dc.title.enMulti-body figures of equilibrium in axial symmetry
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.countryFR
bordeaux.conference.cityBordeaux
bordeaux.peerReviewedoui
hal.identifierhal-01981696
hal.version1
hal.invitednon
hal.proceedingsnon
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01981696v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.date=2018&rft.au=BOUTIN-BASILLAIS,%20B.&HUR%C3%89,%20J.-M.&rft.genre=unknown


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